Origin of Ti-rich garnets in the groundmass of Wajrakarur field kimberlites, southern India: insights from EPMA and Raman spectroscopy
Although Ti-rich garnets are commonly encountered in the groundmass of many alkaline igneous rocks, they are comparatively rare in kimberlites. Here we report on the occurrence of Ti-rich garnets in the groundmass of the P-15 and KL-3 kimberlites from the diamondiferous Wajrakarur field in the Easte...
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description | Although Ti-rich garnets are commonly encountered in the groundmass of many alkaline igneous rocks, they are comparatively rare in kimberlites. Here we report on the occurrence of Ti-rich garnets in the groundmass of the P-15 and KL-3 kimberlites from the diamondiferous Wajrakarur field in the Eastern Dharwar craton of southern India. These garnets contain considerable Ti (11.7–23.9 wt.% TiO
2
), Ca (31.3–35.8 wt.% CaO), Fe (6.8–15.5 wt.% FeO
T
) and Cr (0.04–9.7 wt.% Cr
2
O
3
), but have low Al (0.2–5.7 wt.% Al
2
O
3
). In the case of the P-15 kimberlite they display a range in compositions from andradite to schorlomite, with a low proportion of grossular (andradite
(17.7–49.9)
schorlomite
(34.6–49.5)
-grossular
(3.7–22.8)
-pyrope
(1.9–10.4)
). A few grains also contain significant chromium and represent a solid solution between schorlomite and uvarovite. The Ti-rich garnets in the KL-3 kimberlite, in contrast, are mostly schorlomitic (54.9─90.9 mol %) in composition. The Ti-rich garnets in the groundmass of these two kimberlites are intimately associated with chromian spinels, perhaps suggesting that the garnet formed through the replacement of spinel. From the textural evidence, it appears unlikely that the garnets could have originated through secondary alteration, but rather seem to have formed through a process in which early magmatic spinels have reacted with late circulating, residual fluids in the final stages of crystallization of the kimberlite magma. Raman spectroscopy provides evidence for low crystallinity in the spinels which is likely to be a result of their partial transformation into andradite during their reaction with a late-stage magmatic (kimberlitic) fluid. The close chemical association of these Ti-rich garnets in TiO
2
-FeO-CaO space with those reported from ultramafic lamprophyres (UML) is also consistent with results predicted by experimental studies, and possibly implies a genetic link between kimberlite and UML magmas. The occurrence of Ti-rich garnets of similar composition in the Swartruggens orangeite on the Kaapvaal craton in South Africa, as well as in other kimberlites with an orangeitic affinity (e.g. the P-15 kimberlite on the Eastern Dharwar craton in southern India), is inferred to be a reflection of the high Ca- and high Ti-, and the low Al-nature, of the parent magma (i.e. Group II kimberlites). |
doi_str_mv | 10.1007/s00710-016-0428-4 |
format | Article |
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2
), Ca (31.3–35.8 wt.% CaO), Fe (6.8–15.5 wt.% FeO
T
) and Cr (0.04–9.7 wt.% Cr
2
O
3
), but have low Al (0.2–5.7 wt.% Al
2
O
3
). In the case of the P-15 kimberlite they display a range in compositions from andradite to schorlomite, with a low proportion of grossular (andradite
(17.7–49.9)
schorlomite
(34.6–49.5)
-grossular
(3.7–22.8)
-pyrope
(1.9–10.4)
). A few grains also contain significant chromium and represent a solid solution between schorlomite and uvarovite. The Ti-rich garnets in the KL-3 kimberlite, in contrast, are mostly schorlomitic (54.9─90.9 mol %) in composition. The Ti-rich garnets in the groundmass of these two kimberlites are intimately associated with chromian spinels, perhaps suggesting that the garnet formed through the replacement of spinel. From the textural evidence, it appears unlikely that the garnets could have originated through secondary alteration, but rather seem to have formed through a process in which early magmatic spinels have reacted with late circulating, residual fluids in the final stages of crystallization of the kimberlite magma. Raman spectroscopy provides evidence for low crystallinity in the spinels which is likely to be a result of their partial transformation into andradite during their reaction with a late-stage magmatic (kimberlitic) fluid. The close chemical association of these Ti-rich garnets in TiO
2
-FeO-CaO space with those reported from ultramafic lamprophyres (UML) is also consistent with results predicted by experimental studies, and possibly implies a genetic link between kimberlite and UML magmas. The occurrence of Ti-rich garnets of similar composition in the Swartruggens orangeite on the Kaapvaal craton in South Africa, as well as in other kimberlites with an orangeitic affinity (e.g. the P-15 kimberlite on the Eastern Dharwar craton in southern India), is inferred to be a reflection of the high Ca- and high Ti-, and the low Al-nature, of the parent magma (i.e. Group II kimberlites).</description><identifier>ISSN: 0930-0708</identifier><identifier>EISSN: 1438-1168</identifier><identifier>DOI: 10.1007/s00710-016-0428-4</identifier><language>eng</language><publisher>Vienna: Springer Vienna</publisher><subject>Chromium ; Cratons ; Crystallization ; Earth and Environmental Science ; Earth Sciences ; Garnets ; Geochemistry ; Igneous rocks ; India ; Inorganic Chemistry ; Magma ; Mineralogy ; Original Paper ; Spectroscopy ; Spectrum analysis ; Spinel ; Titanium ; Titanium dioxide</subject><ispartof>Mineralogy and petrology, 2016-04, Vol.110 (2-3), p.295-307</ispartof><rights>Springer-Verlag Wien 2016</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a471t-151be14f06bc6c79decadf520b411ed60cdf3dafff4fbb8c177fcc3b3a23b33e3</citedby><cites>FETCH-LOGICAL-a471t-151be14f06bc6c79decadf520b411ed60cdf3dafff4fbb8c177fcc3b3a23b33e3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s00710-016-0428-4$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s00710-016-0428-4$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Dongre, Ashish N.</creatorcontrib><creatorcontrib>Viljoen, K. S.</creatorcontrib><creatorcontrib>Rao, N. V. Chalapathi</creatorcontrib><creatorcontrib>Gucsik, A.</creatorcontrib><title>Origin of Ti-rich garnets in the groundmass of Wajrakarur field kimberlites, southern India: insights from EPMA and Raman spectroscopy</title><title>Mineralogy and petrology</title><addtitle>Miner Petrol</addtitle><description>Although Ti-rich garnets are commonly encountered in the groundmass of many alkaline igneous rocks, they are comparatively rare in kimberlites. Here we report on the occurrence of Ti-rich garnets in the groundmass of the P-15 and KL-3 kimberlites from the diamondiferous Wajrakarur field in the Eastern Dharwar craton of southern India. These garnets contain considerable Ti (11.7–23.9 wt.% TiO
2
), Ca (31.3–35.8 wt.% CaO), Fe (6.8–15.5 wt.% FeO
T
) and Cr (0.04–9.7 wt.% Cr
2
O
3
), but have low Al (0.2–5.7 wt.% Al
2
O
3
). In the case of the P-15 kimberlite they display a range in compositions from andradite to schorlomite, with a low proportion of grossular (andradite
(17.7–49.9)
schorlomite
(34.6–49.5)
-grossular
(3.7–22.8)
-pyrope
(1.9–10.4)
). A few grains also contain significant chromium and represent a solid solution between schorlomite and uvarovite. The Ti-rich garnets in the KL-3 kimberlite, in contrast, are mostly schorlomitic (54.9─90.9 mol %) in composition. The Ti-rich garnets in the groundmass of these two kimberlites are intimately associated with chromian spinels, perhaps suggesting that the garnet formed through the replacement of spinel. From the textural evidence, it appears unlikely that the garnets could have originated through secondary alteration, but rather seem to have formed through a process in which early magmatic spinels have reacted with late circulating, residual fluids in the final stages of crystallization of the kimberlite magma. Raman spectroscopy provides evidence for low crystallinity in the spinels which is likely to be a result of their partial transformation into andradite during their reaction with a late-stage magmatic (kimberlitic) fluid. The close chemical association of these Ti-rich garnets in TiO
2
-FeO-CaO space with those reported from ultramafic lamprophyres (UML) is also consistent with results predicted by experimental studies, and possibly implies a genetic link between kimberlite and UML magmas. The occurrence of Ti-rich garnets of similar composition in the Swartruggens orangeite on the Kaapvaal craton in South Africa, as well as in other kimberlites with an orangeitic affinity (e.g. the P-15 kimberlite on the Eastern Dharwar craton in southern India), is inferred to be a reflection of the high Ca- and high Ti-, and the low Al-nature, of the parent magma (i.e. Group II kimberlites).</description><subject>Chromium</subject><subject>Cratons</subject><subject>Crystallization</subject><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Garnets</subject><subject>Geochemistry</subject><subject>Igneous rocks</subject><subject>India</subject><subject>Inorganic Chemistry</subject><subject>Magma</subject><subject>Mineralogy</subject><subject>Original Paper</subject><subject>Spectroscopy</subject><subject>Spectrum analysis</subject><subject>Spinel</subject><subject>Titanium</subject><subject>Titanium dioxide</subject><issn>0930-0708</issn><issn>1438-1168</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>8G5</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><sourceid>GUQSH</sourceid><sourceid>M2O</sourceid><recordid>eNqNkctqHDEQRYVJIBMnH5CdwBsv0k5VPzXZGePEBgeb4JClUOvRo3G3NFZ1L_wD-W5rGC-CIZBNFZTOvVTpMvYJ4QwBui-UC0IB2BZQl6Koj9gK60oUiK14w1awrvJrB-Ide0-0BQDRCFyxP7fJDz7w6Pi9L5LXGz6oFOxMPE_njeVDikswkyLaQ7_VNqkHlZbEnbej4Q9-6m0a_WzpM6e4ZEkK_DoYr75mC_LDJnu5FCd-effjnKtg-E81qcBpZ_WcIum4e_rA3jo1kv340o_Zr2-X9xdXxc3t9-uL85tC1R3OBTbYW6wdtL1udbc2VivjmhL6GtGaFrRxlVHOudr1vdDYdU7rqq9UmUtlq2N2evDdpfi4WJrl5EnbcVTBxoUkChDQdGW5_h-0abDsUGT05BW6jUsK-RCZN2iq_Ndlmyk8UDofTck6uUt-UulJIsh9iPIQoswhyn2Iss6a8qChzIbBpr-c_yl6BiskoOA</recordid><startdate>20160401</startdate><enddate>20160401</enddate><creator>Dongre, Ashish N.</creator><creator>Viljoen, K. S.</creator><creator>Rao, N. V. Chalapathi</creator><creator>Gucsik, A.</creator><general>Springer Vienna</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7XB</scope><scope>88I</scope><scope>8BQ</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>8G5</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ATCPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>CCPQU</scope><scope>D1I</scope><scope>DWQXO</scope><scope>F1W</scope><scope>FR3</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H96</scope><scope>HCIFZ</scope><scope>JG9</scope><scope>KB.</scope><scope>KR7</scope><scope>L.G</scope><scope>L6V</scope><scope>M2O</scope><scope>M2P</scope><scope>M7S</scope><scope>MBDVC</scope><scope>PATMY</scope><scope>PCBAR</scope><scope>PDBOC</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PTHSS</scope><scope>PYCSY</scope><scope>Q9U</scope><scope>7UA</scope><scope>C1K</scope></search><sort><creationdate>20160401</creationdate><title>Origin of Ti-rich garnets in the groundmass of Wajrakarur field kimberlites, southern India: insights from EPMA and Raman spectroscopy</title><author>Dongre, Ashish N. ; Viljoen, K. S. ; Rao, N. V. Chalapathi ; Gucsik, A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a471t-151be14f06bc6c79decadf520b411ed60cdf3dafff4fbb8c177fcc3b3a23b33e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Chromium</topic><topic>Cratons</topic><topic>Crystallization</topic><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Garnets</topic><topic>Geochemistry</topic><topic>Igneous rocks</topic><topic>India</topic><topic>Inorganic Chemistry</topic><topic>Magma</topic><topic>Mineralogy</topic><topic>Original Paper</topic><topic>Spectroscopy</topic><topic>Spectrum analysis</topic><topic>Spinel</topic><topic>Titanium</topic><topic>Titanium dioxide</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Dongre, Ashish N.</creatorcontrib><creatorcontrib>Viljoen, K. S.</creatorcontrib><creatorcontrib>Rao, N. 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Chalapathi</creatorcontrib><creatorcontrib>Gucsik, A.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>METADEX</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>Research Library (Alumni Edition)</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Agricultural & Environmental Science Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Materials Science Collection</collection><collection>ProQuest Central Korea</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Engineering Research Database</collection><collection>ProQuest Central Student</collection><collection>Research Library Prep</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>SciTech Premium Collection</collection><collection>Materials Research Database</collection><collection>Materials Science Database</collection><collection>Civil Engineering Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>ProQuest Engineering Collection</collection><collection>Research Library</collection><collection>Science Database</collection><collection>Engineering Database</collection><collection>Research Library (Corporate)</collection><collection>Environmental Science Database</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>Materials Science Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>Engineering Collection</collection><collection>Environmental Science Collection</collection><collection>ProQuest Central Basic</collection><collection>Water Resources Abstracts</collection><collection>Environmental Sciences and Pollution Management</collection><jtitle>Mineralogy and petrology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Dongre, Ashish N.</au><au>Viljoen, K. S.</au><au>Rao, N. V. Chalapathi</au><au>Gucsik, A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Origin of Ti-rich garnets in the groundmass of Wajrakarur field kimberlites, southern India: insights from EPMA and Raman spectroscopy</atitle><jtitle>Mineralogy and petrology</jtitle><stitle>Miner Petrol</stitle><date>2016-04-01</date><risdate>2016</risdate><volume>110</volume><issue>2-3</issue><spage>295</spage><epage>307</epage><pages>295-307</pages><issn>0930-0708</issn><eissn>1438-1168</eissn><abstract>Although Ti-rich garnets are commonly encountered in the groundmass of many alkaline igneous rocks, they are comparatively rare in kimberlites. Here we report on the occurrence of Ti-rich garnets in the groundmass of the P-15 and KL-3 kimberlites from the diamondiferous Wajrakarur field in the Eastern Dharwar craton of southern India. These garnets contain considerable Ti (11.7–23.9 wt.% TiO
2
), Ca (31.3–35.8 wt.% CaO), Fe (6.8–15.5 wt.% FeO
T
) and Cr (0.04–9.7 wt.% Cr
2
O
3
), but have low Al (0.2–5.7 wt.% Al
2
O
3
). In the case of the P-15 kimberlite they display a range in compositions from andradite to schorlomite, with a low proportion of grossular (andradite
(17.7–49.9)
schorlomite
(34.6–49.5)
-grossular
(3.7–22.8)
-pyrope
(1.9–10.4)
). A few grains also contain significant chromium and represent a solid solution between schorlomite and uvarovite. The Ti-rich garnets in the KL-3 kimberlite, in contrast, are mostly schorlomitic (54.9─90.9 mol %) in composition. The Ti-rich garnets in the groundmass of these two kimberlites are intimately associated with chromian spinels, perhaps suggesting that the garnet formed through the replacement of spinel. From the textural evidence, it appears unlikely that the garnets could have originated through secondary alteration, but rather seem to have formed through a process in which early magmatic spinels have reacted with late circulating, residual fluids in the final stages of crystallization of the kimberlite magma. Raman spectroscopy provides evidence for low crystallinity in the spinels which is likely to be a result of their partial transformation into andradite during their reaction with a late-stage magmatic (kimberlitic) fluid. The close chemical association of these Ti-rich garnets in TiO
2
-FeO-CaO space with those reported from ultramafic lamprophyres (UML) is also consistent with results predicted by experimental studies, and possibly implies a genetic link between kimberlite and UML magmas. The occurrence of Ti-rich garnets of similar composition in the Swartruggens orangeite on the Kaapvaal craton in South Africa, as well as in other kimberlites with an orangeitic affinity (e.g. the P-15 kimberlite on the Eastern Dharwar craton in southern India), is inferred to be a reflection of the high Ca- and high Ti-, and the low Al-nature, of the parent magma (i.e. Group II kimberlites).</abstract><cop>Vienna</cop><pub>Springer Vienna</pub><doi>10.1007/s00710-016-0428-4</doi><tpages>13</tpages></addata></record> |
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subjects | Chromium Cratons Crystallization Earth and Environmental Science Earth Sciences Garnets Geochemistry Igneous rocks India Inorganic Chemistry Magma Mineralogy Original Paper Spectroscopy Spectrum analysis Spinel Titanium Titanium dioxide |
title | Origin of Ti-rich garnets in the groundmass of Wajrakarur field kimberlites, southern India: insights from EPMA and Raman spectroscopy |
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